CWNU 349

0.16 UTI

0.54

C_N

0.47

C_dens

0.75

C_C3

0.0

C_lit

0.47

C_dup

N_m (P>50%) 58

Core radius and density 1.5 [pc], 2.4 [pc^-2]

C3 classification AB

C_N 0.54 Moderately populated
C_dens 0.47 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.47 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 349 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 349 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	306.686	49.117	0.585	0.176	-3.857	-4.05
He et al.	2022	306.668	49.117	0.59	0.17	-3.86	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	2.0	1.46	–	631	0.374	–	–	–
He et al.	2022	2.00	1.46	–	631	0.374	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1116	53.4	306.69	49.12	0.59	0.17	-3.86	-4.05	0.38
CWWDL 13016	43.1	306.69	49.12	0.59	0.18	-3.86	-4.05	0.0

💡 Note: The % column shows the percentage of members that CWNU 349 shares with each listed object.

Visualization

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